By combining effective field theory with the standard nuclear physics approach (SNPA) we obtain a high-precision estimate of the $S$ factor for the solar $hep$ process. The accurate wave functions available in SNPA are used to evaluate the nuclear matrix elements for the transition operators that result from chiral perturbation theory (ChPT). All the contributions up to \nlo3 in ChPT are included. The resulting parameter-free, error-controlled prediction is: $S(hep)=(8.6 \pm 1.3)\times 10^{-20}$ keV-b
The astrophysical S factor for the proton weak capture on 3He is calculated with correlated-hypersph...
We compute the S-factor of the proton-proton (pp) fusion reaction using chiral effective field theor...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to ${\ca...
Using effective field theory, we calculate the S-factor for the hep process in a totally parameter-f...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to {Omic...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to ${\ca...
Recently we succeeded to make a reliable EFT prediction in a totally parameter-free manner for the $...
We discuss the problem of solar hep neutrinos originating from the reaction p+ 3He -> 4He + e+ + nu ...
The results of a new calculation of the astrophysical S-factor for the proton weak capture on 3He ar...
The astrophysical factor for the proton weak capture on 3He is calculated with correlated-hyperspher...
AbstractThe cross sections for low-energy neutrino–deuteron reactions are calculated within heavy-ba...
Key Words solar burning, solar neutrinos, neutrino oscillations, effective field theory PACS Codes 2...
High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He with a large end point...
We discuss microscopic cluster model descriptions of two solar nuclear reactions, Be7(p,gamma)B8 and...
The astrophysical S factor for the proton weak capture on 3He is calculated with correlated-hypersph...
We compute the S-factor of the proton-proton (pp) fusion reaction using chiral effective field theor...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to ${\ca...
Using effective field theory, we calculate the S-factor for the hep process in a totally parameter-f...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to {Omic...
Spurred by the recent complete determination of the weak currents in two-nucleon systems up to ${\ca...
Recently we succeeded to make a reliable EFT prediction in a totally parameter-free manner for the $...
We discuss the problem of solar hep neutrinos originating from the reaction p+ 3He -> 4He + e+ + nu ...
The results of a new calculation of the astrophysical S-factor for the proton weak capture on 3He ar...
The astrophysical factor for the proton weak capture on 3He is calculated with correlated-hyperspher...
AbstractThe cross sections for low-energy neutrino–deuteron reactions are calculated within heavy-ba...
Key Words solar burning, solar neutrinos, neutrino oscillations, effective field theory PACS Codes 2...
High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He with a large end point...
We discuss microscopic cluster model descriptions of two solar nuclear reactions, Be7(p,gamma)B8 and...
The astrophysical S factor for the proton weak capture on 3He is calculated with correlated-hypersph...
We compute the S-factor of the proton-proton (pp) fusion reaction using chiral effective field theor...
The astrophysical factor for the proton weak capture on {sup 3}He is calculated with correlated-hype...